A new public code (SIRIO) predicts that reconnection-driven star-planet interaction can explain tentative radio detections from Proxima, YZ Ceti, and GJ 1151, while Alfvén-wing emission is too faint and free-free absorption is significant at high mass-loss rates.
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Modelling magnetic star-planet interaction in the iconic M dwarfs Proxima Centauri, YZ Ceti and GJ 1151
A new public code (SIRIO) predicts that reconnection-driven star-planet interaction can explain tentative radio detections from Proxima, YZ Ceti, and GJ 1151, while Alfvén-wing emission is too faint and free-free absorption is significant at high mass-loss rates.